Disc instability models for X-ray transients: Evidence for evaporation and low α-viscosity?

Monthly Notices of the Royal Astronomical Society

Volumn 314, Issue 3, 2000, Pages 498-510

  Menou, Kristen ^a,b,c,f   Hameury, Jean Marie ^c,d   Lasota, Jean Pierre ^b,c,e   Narayan, Ramesh ^a,c  

^a HARVARD SMITHSONIAN CENTER FOR ASTROPHYSICS   (United States)

^b OBSERVATOIRE DE PARIS   (France)

^c UNIVERSITY OF CALIFORNIA   (United States)

^d OBSERVATOIRE DE STRASBOURG   (France)

^e INSTITUT D'ASTROPHYSIQUE DE PARIS   (France)

^f PRINCETON UNIVERSITY   (United States)

Author keywords

Accretion, accretion discs; Black hole physics; MHD; Novae, cataclysmic variables; Turbulence; X rays: Stars

Indexed keywords

BLACK HOLES; GRAVITATION; IRRADIATION; STARS; VISCOSITY;

ACCRETION DISCS; ACCRETION: ACCRETION DISKS; BLACK HOLE PHYSICS; DISK INSTABILITIES; INSTABILITY MODEL; NOVAE CATACLYSMIC VARIABLES; RECURRENCE TIME; TIME-DEPENDENT MODELS; X-RAY TRANSIENTS; X-RAY:STARS;

EVAPORATION;

EID: 0000135418     PISSN: 00358711     EISSN: None     Source Type: Journal    
DOI: 10.1046/j.1365-8711.2000.03357.x     Document Type: Article

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